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Titel Observation of a lunar mini-magnetosphere above a magnetic anomaly using energetic neutral atoms
VerfasserIn Martin Wieser, Stas Barabash, Yoshifumi Futaana, Mats Holmström, Anil Bhardwaj, R. Sridharan, M. B. Dhanya, Audrey Schaufelberger, Peter Wurz, Kazushi Asamura
Konferenz EGU General Assembly 2010
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 12 (2010)
Datensatznummer 250039163
 
Zusammenfassung
The Sub-keV Atom Reflecting Analyzer (SARA) instrument on the Indian Chandrayaan-1 spacecraft has resulted in a comprehensive data set about interaction of solar wind with the lunar surface. When solar wind hits the lunar surface, it is partly backscattered as energetic neutral atoms. The intensity of the backscattered energetic neutral atoms is a measure of the intensity of the solar wind reaching the surface. We report on the imaging of a lunar magnetic anomaly in backscattered neutral hydrogen atoms: The image shows the formation of a partial void of the solar wind, a mini-magnetosphere, above the strong magnetic anomaly near the Crisium antipode on the lunar farside. The mini-magnetosphere is 360 km across at the surface and surrounded by a 300-km-thick region of enhanced plasma flux that results from the solar wind flowing around the mini-magnetosphere. These observations demonstrate a new observational technique to study airless bodies, imaging in backscattered neutral atoms, and its application to a new class of objects, mini-magnetospheres.